CWWDL 2701

0.06 UTI

0.64

C_N

1.0

C_dens

0.62

C_C3

0.0

C_lit

0.13

C_dup

C3 classification CA

Number of members (P>50%) 77

Radius (P>50% members) 2.5 [arcmin]

C_N 0.64 Moderately populated
C_dens 1.0 Very dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.13 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWWDL 2701 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Near-solar metallicity Intermediate age

Data

🔍 Search references for CWWDL 2701 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	122.505	-29.851	0.204	-2.767	2.6	59.568
Chi et al.	2023	122.475	-29.848	0.228	-2.64	2.555	57.584

💡 Note: The UCC values are estimated from its identified members.

Reference	Year	Dist [kpc]	Av [mag]	DAv [mag]	Age [Myr]	[Fe/H] [dex]	Mass [Msun]	Bfr	BSS
Chi et al.	2023	–	–	–	115	0.420	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 2661	87.0	122.51	-29.85	0.21	-2.79	2.63	58.83	0.58

💡 Note: The % column shows the percentage of members that CWWDL 2701 shares with each listed object.

Visualization

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